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New Last Glacial Maximum Ice Thickness Constraints for The Edinburgh Research Explorer New Last Glacial Maximum Ice Thickness constraints for the Weddell Sea Embayment, Antarctica Citation for published version: Nichols, KA, Goehring, BM, Balco, G, Johnson, JS, Hein, A & Todd, C 2019, 'New Last Glacial Maximum Ice Thickness constraints for the Weddell Sea Embayment, Antarctica', Cryosphere. https://doi.org/10.5194/tc-13-2935-2019 Digital Object Identifier (DOI): 10.5194/tc-13-2935-2019 Link: Link to publication record in Edinburgh Research Explorer Document Version: Publisher's PDF, also known as Version of record Published In: Cryosphere Publisher Rights Statement: © Author(s) 2019. This work is distributed under the Creative Commons Attribution 4.0 License. General rights Copyright for the publications made accessible via the Edinburgh Research Explorer is retained by the author(s) and / or other copyright owners and it is a condition of accessing these publications that users recognise and abide by the legal requirements associated with these rights. Take down policy The University of Edinburgh has made every reasonable effort to ensure that Edinburgh Research Explorer content complies with UK legislation. If you believe that the public display of this file breaches copyright please contact [email protected] providing details, and we will remove access to the work immediately and investigate your claim. Download date: 09. Oct. 2021 The Cryosphere, 13, 2935–2951, 2019 https://doi.org/10.5194/tc-13-2935-2019 © Author(s) 2019. This work is distributed under the Creative Commons Attribution 4.0 License. New Last Glacial Maximum ice thickness constraints for the Weddell Sea Embayment, Antarctica Keir A. Nichols1, Brent M. Goehring1, Greg Balco2, Joanne S. Johnson3, Andrew S. Hein4, and Claire Todd5 1Department of Earth and Environmental Sciences, Tulane University, New Orleans, LA 70118, USA 2Berkeley Geochronology Center, 2455 Ridge Road, Berkeley, CA 94709, USA 3British Antarctic Survey, Natural Environment Research Council, High Cross, Madingley Road, Cambridge, CB3 0ET, UK 4School of GeoSciences, University of Edinburgh, Drummund Street, Edinburgh, EH8 9XP, UK 5Department of Geosciences, Pacific Lutheran University, Tacoma, WA 98447, USA Correspondence: Keir A. Nichols ([email protected]) Received: 27 March 2019 – Discussion started: 14 May 2019 Revised: 12 September 2019 – Accepted: 2 October 2019 – Published: 8 November 2019 Abstract. We describe new Last Glacial Maximum (LGM) surements indicate that the long-lived nuclide measurements ice thickness constraints for three locations spanning the of previous studies were influenced by cosmogenic nuclide Weddell Sea Embayment (WSE) of Antarctica. Samples col- inheritance. Our inferred LGM configuration, which is pri- lected from the Shackleton Range, Pensacola Mountains, and marily based on minimum ice thickness constraints and thus the Lassiter Coast constrain the LGM thickness of the Slessor does not constrain an upper limit, indicates a relatively mod- Glacier, Foundation Ice Stream, and grounded ice proximal est contribution to sea level rise since the LGM of < 4.6 m, to the modern Ronne Ice Shelf edge on the Antarctic Penin- and possibly as little as < 1.5 m. sula, respectively. Previous attempts to reconstruct LGM-to- present ice thickness changes around the WSE used measure- ments of long-lived cosmogenic nuclides, primarily 10Be. An absence of post-LGM apparent exposure ages at many 1 Introduction sites led to LGM thickness reconstructions that were spatially highly variable and inconsistent with flow line modelling. Es- We describe new constraints on Last Glacial Maximum timates for the contribution of the ice sheet occupying the (LGM, ca. 26 to 15 ka; Peltier and Fairbanks, 2006) ice WSE at the LGM to global sea level since deglaciation vary thickness changes from three locations within the Weddell by an order of magnitude, from 1.4 to 14.1 m of sea level Sea Embayment (WSE) of Antarctica (Fig. 1). The WSE equivalent. Here we use a short-lived cosmogenic nuclide, drains approximately one-fifth of the total area of the Antarc- in situ-produced 14C, which is less susceptible to inheritance tic ice sheets (AISs) (Joughin et al., 2006) and is thus an problems than 10Be and other long-lived nuclides. We use important contributor to LGM-to-present and, potentially, in situ 14C to evaluate the possibility that sites with no post- future sea level change. Previous attempts to reconstruct LGM exposure ages are biased by cosmogenic nuclide inher- LGM-to-present ice thickness changes around the WSE used itance due to surface preservation by cold-based ice and non- measurements of long-lived cosmogenic nuclides, primarily deposition of LGM-aged drift. Our measurements show that 10Be (half-life 1:387 ± 0:012 Ma; Chmeleff et al., 2010; Ko- the Slessor Glacier was between 310 and up to 655 m thicker rschinek et al., 2010) and 26Al (half-life 705 ± 17 ka; Nor- than present at the LGM. The Foundation Ice Stream was at ris et al., 1983), sourced from bedrock and erratic cobbles least 800 m thicker, and ice on the Lassiter Coast was at least proximal to modern glacier surfaces. Through measuring the 385 m thicker than present at the LGM. With evidence for cosmogenic nuclide concentration of samples of glacial de- LGM thickening at all of our study sites, our in situ 14C mea- posits and bedrock, one can constrain the magnitude and tim- ing of past changes in the thickness of adjacent ice masses. Published by Copernicus Publications on behalf of the European Geosciences Union. 2936 K. A. Nichols et al.: LGM ice thickness constraints for the Weddell Sea Embayment However, an absence of post-LGM apparent exposure ages at many sites around the WSE led to LGM thickness recon- structions that were spatially highly variable and inconsis- tent with flow line modelling (e.g. Whitehouse et al., 2017). Consequently, estimates based on ice models constrained by field evidence (Le Brocq et al., 2011) and by relative sea level records and earth viscosity models (Bassett et al., 2007) for the contribution of the sector to global sea level since deglaciation began vary by an order of magnitude, from 1.4 to 14.1 m, respectively. The lack of geological evidence for LGM thickening is also manifest in a misfit between present- day geodetic uplift rate measurements in southern Palmer Land and predicted uplift rates from a glacial isostatic adjust- ment (GIA) model (Wolstencroft et al., 2015). Constraining the previous vertical extent of ice provides inputs to numer- ical models investigating both the response of the ice sheet to past and potential future changes in climate and sea level (e.g. Briggs et al., 2014; Pollard et al., 2016, 2017; White- house et al., 2017) as well as the response of the solid earth to past ice load changes to quantify present-day ice-mass loss (e.g. Wolstencroft et al., 2015). Furthermore, quantify- ing the LGM dimensions of the WSE sector of the AIS is Figure 1. The Weddell Sea Embayment, including all locations required to further constrain the offset between estimates for referred to within the text. SH, WH, and TH are the Schmidt, post-LGM sea level rise and estimates of the total amount of Williams, and Thomas Hills, respectively. FH, P/M, and MH are ice melted since the LGM. The former is sourced from sea the Flower Hills, Patriot and Marble Hills, and the Meyer Hills, re- level index points, and the latter is sourced from our knowl- spectively. Black is exposed rock. Red boxes show extent of satel- edge of the dimensions of ice masses at the LGM (Simms et lite images in Fig. 4. Exposed rock and coastline sourced from the al., 2019). Currently, the “missing ice” accounts for between SCAR Antarctic Digital Database. Bathymetry sourced from the 15:6 ± 9:6 and 18:1 ± 9:6 m of global sea level rise since the International Bathymetric Chart of the Southern Ocean V1.0 (IB- SCO; Arndt et al., 2013). Surface topography (shading) is sourced LGM (Simms et al., 2019). from the Reference Elevation Model of Antarctica (REMA; Howat Although the use of cosmogenic nuclide geochronology et al., 2019). PS1423-2 is a marine sediment core from Crawford et to study the AIS is clearly proven (e.g. Stone et al., 2003; al. (1996). Ackert et al., 2007), applications in the WSE are challeng- ing. Many studies, despite making multiple cosmogenic nu- clide measurements from relatively large numbers of sam- ples, observed no or few post-LGM exposure ages (Hein et burial (e.g. Bentley et al., 2006; Sugden et al., 2017). Cold- al., 2011, 2014; Balco et al., 2016; Bentley et al., 2017). With based ice preserves surfaces (e.g. Stroeven et al., 2002; Sug- no evidence for LGM ice cover, it was not clear whether den et al., 2005; Gjermundsen et al., 2015), allowing nuclide sites were covered by ice at the LGM, or whether sites were concentrations to persist within surfaces from previous peri- covered but the ice left no fresh deposits on top of those ods of exposure to the present, a phenomenon known as in- yielding pre-LGM ages. It is therefore currently unknown heritance. Long-lived nuclides are particularly susceptible to whether ice was thicker than present during the LGM at the inheritance due to their long half-lives which, when protected Schmidt Hills in the Pensacola Mountains and in the Shack- from erosion beneath cold-based ice, require long periods of leton Range (Figs. 1 and 2). Results from the Schmidt Hills burial to reduce concentrations to below measurable levels. (Fig. 2) indicating no LGM thickening of the Foundation When covered by cold-based ice during glaciations, concen- Ice Stream (FIS) are particularly problematic, as thicken- trations of long-lived nuclides record exposure during multi- ing of 500 m from the Williams Hills, 50 km upstream of ple separate ice-free periods rather than just the most recent the Schmidt Hills, produces a LGM surface slope that is one.
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